We take our target list of globular clusters from [1]}. To this sample we add six additional Milky Way globular clusters that have been found in recent years:
VVV-CL001 [2]}, [3]}, BH 140 and FSR 1758 [4]}, Sagittarius II [5]}, [6]}, RLGC 1 and RLGC 2 [7]}, and
Laevens 3 [8]}. The status of Sagittarius II is still debated, while [6]} argue for it to be a star cluster based on its location in a size vs.
luminosity plane, [10]} argue,
based on a small spread in [Fe/H] that they find among the cluster stars, for it to be a dwarf galaxy. We tentatively include the object in our list of clusters. The other systems are most likely globular clusters based
on their color-magnitude diagrams, kinematics and location in the Milky Way. Together with the 158 GCs studied in [1]}, we therefore have a sample of 162 globular clusters.
